Fig. 1.
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Middle: comparison between zphot and zspec in the sample of selected EELGs. The dashed black line is the 1:1 relation. Right: distribution of zspec, shown as superimposed histograms. In both panels, in red (blue), the galaxies with PRISM (MR) spectra. Top: distribution of zphot in the photometric parent sample (Llerena et al. 2024).
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